Difference between revisions of "LPOD June 11, 2008"

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[[Image:LPOD-June11-08.jpg|LPOD-June11-08.jpg]]<br /> ''figure compiled from [http://www.christian-woehler.de/undarum_pss.pdf Lunar domes in Mare Undarum: Spectral and morphometric properties, eruption conditions, and mode of emplacement]''<br /> <br />  For the last 60 years the distinction between amateur and professional observers of the Moon was clear. Amateurs made visual and imaging observations and commented on the smallness of detected features. Professional observers made measurements and physical models. [http://www2.lpod.org/wiki/January_8,_2004 Ralph Baldwin] was one of the earliest modern professionals, measuring crater diameters and depths to compare with volcanic and explosion craters on Earth. Later, telescopic and then spacecraft spectral data provided a powerful tool to quantitatively distinguish - and sometimes identify - compositions of different lunar materials. Most amateurs today still just observe and image - and that is OK for they are like serious tourists seeking to understand a strange land. Others, who started out as tourists, have made the transition to professional status because of their measurements and modeling. The most successful example are members of the [http://www.glrgroup.org/home.htm the Geological Lunar Research Group] who have specialized in understanding the physical conditions and processes of lunar dome eruptions. Their latest [http://www.christian-woehler.de/undarum_pss.pdf paper] concerns these domes in Mare Undarum, north and east of the lava-floored crater Dubiago. The top four domes, labeled Co1 to Co4 after the nearby Condorcet crater, are somewhat traditional domes about 10-12 km in diameter, with Co4 having a greater height, and thus volume and slope, than its neighbors. The dome Du3 is about the same diameter, but much less steep (~0.9°) and more like a swell than a classical dome. The top table gives these measured quantities, and the bottom table shows the derived ones from models of magma rise and eruption. One of the most interesting - and understandable - quantities is Te, the inferred duration of eruption, which ranges from 3 months to nearly 5 years. Careful perusers will note that the eruption durations are proportional to erupted volumes, which makes sense. To find out what all the other columns of data mean see the full [http://www.christian-woehler.de/undarum_pss.pdf paper] by Raffeallo Lena and his coauthors. [http://www.christian-woehler.de/lunar_dem.html Here] is a general overview of this professional work on domes. Note that these Undarum results are based on images by people well known to LPOD readers: Stefan Lammel, Paolo Lazzarotti and Bob Pilz, and coordinates were determined using Jim Mosher's [http://ltvt.wikispaces.com/LTVT LTVT] software. <br /> <br /> ''Chuck Wood''<br /> <br /> '''Related Links'''<br />  Rükl plate 38<br /> <br /> <br />
 
[[Image:LPOD-June11-08.jpg|LPOD-June11-08.jpg]]<br /> ''figure compiled from [http://www.christian-woehler.de/undarum_pss.pdf Lunar domes in Mare Undarum: Spectral and morphometric properties, eruption conditions, and mode of emplacement]''<br /> <br />  For the last 60 years the distinction between amateur and professional observers of the Moon was clear. Amateurs made visual and imaging observations and commented on the smallness of detected features. Professional observers made measurements and physical models. [http://www2.lpod.org/wiki/January_8,_2004 Ralph Baldwin] was one of the earliest modern professionals, measuring crater diameters and depths to compare with volcanic and explosion craters on Earth. Later, telescopic and then spacecraft spectral data provided a powerful tool to quantitatively distinguish - and sometimes identify - compositions of different lunar materials. Most amateurs today still just observe and image - and that is OK for they are like serious tourists seeking to understand a strange land. Others, who started out as tourists, have made the transition to professional status because of their measurements and modeling. The most successful example are members of the [http://www.glrgroup.org/home.htm the Geological Lunar Research Group] who have specialized in understanding the physical conditions and processes of lunar dome eruptions. Their latest [http://www.christian-woehler.de/undarum_pss.pdf paper] concerns these domes in Mare Undarum, north and east of the lava-floored crater Dubiago. The top four domes, labeled Co1 to Co4 after the nearby Condorcet crater, are somewhat traditional domes about 10-12 km in diameter, with Co4 having a greater height, and thus volume and slope, than its neighbors. The dome Du3 is about the same diameter, but much less steep (~0.9°) and more like a swell than a classical dome. The top table gives these measured quantities, and the bottom table shows the derived ones from models of magma rise and eruption. One of the most interesting - and understandable - quantities is Te, the inferred duration of eruption, which ranges from 3 months to nearly 5 years. Careful perusers will note that the eruption durations are proportional to erupted volumes, which makes sense. To find out what all the other columns of data mean see the full [http://www.christian-woehler.de/undarum_pss.pdf paper] by Raffeallo Lena and his coauthors. [http://www.christian-woehler.de/lunar_dem.html Here] is a general overview of this professional work on domes. Note that these Undarum results are based on images by people well known to LPOD readers: Stefan Lammel, Paolo Lazzarotti and Bob Pilz, and coordinates were determined using Jim Mosher's [http://ltvt.wikispaces.com/LTVT LTVT] software. <br /> <br /> ''Chuck Wood''<br /> <br /> '''Related Links'''<br />  Rükl plate 38<br /> <br /> <br />
 
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'''COMMENTS'''<br /> <span style="FONT-SIZE: 80%">To [/LPOD%20Comments post comments] regarding this LPOD you need to first register for the wiki by clicking the "Join this space" link under the Full Moon icon in the upper left corner of the screen, and wait for your membership to be approved. Once registered, you may still need to "Sign In" (link at top right of screen) to remove the "Protected" icon from the top of the LPOD page. Once you don't see a "Protected" icon, please click [http://the-moon.us/wiki/page/edit/LPOD+June+11,+2008 here] and enter your comment in the space below. ''Please do not edit the LPOD itself!''</span><br /> <br />  1.<br /> <br /> <br /> <br />
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'''COMMENTS'''<br /> <span style="FONT-SIZE: 80%">To [[LPOD%20Comments|post comments]] regarding this LPOD you need to first register for the wiki by clicking the "Join this space" link under the Full Moon icon in the upper left corner of the screen, and wait for your membership to be approved. Once registered, you may still need to "Sign In" (link at top right of screen) to remove the "Protected" icon from the top of the LPOD page. Once you don't see a "Protected" icon, please click [http://the-moon.us/wiki/page/edit/LPOD+June+11,+2008 here] and enter your comment in the space below. ''Please do not edit the LPOD itself!''</span><br /> <br />  1.<br /> <br /> <br /> <br />
 
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Latest revision as of 14:57, 15 April 2018

LEARNING A LOT ABOUT LITTLE HILLS

LPOD-June11-08.jpg
figure compiled from Lunar domes in Mare Undarum: Spectral and morphometric properties, eruption conditions, and mode of emplacement

For the last 60 years the distinction between amateur and professional observers of the Moon was clear. Amateurs made visual and imaging observations and commented on the smallness of detected features. Professional observers made measurements and physical models. Ralph Baldwin was one of the earliest modern professionals, measuring crater diameters and depths to compare with volcanic and explosion craters on Earth. Later, telescopic and then spacecraft spectral data provided a powerful tool to quantitatively distinguish - and sometimes identify - compositions of different lunar materials. Most amateurs today still just observe and image - and that is OK for they are like serious tourists seeking to understand a strange land. Others, who started out as tourists, have made the transition to professional status because of their measurements and modeling. The most successful example are members of the the Geological Lunar Research Group who have specialized in understanding the physical conditions and processes of lunar dome eruptions. Their latest paper concerns these domes in Mare Undarum, north and east of the lava-floored crater Dubiago. The top four domes, labeled Co1 to Co4 after the nearby Condorcet crater, are somewhat traditional domes about 10-12 km in diameter, with Co4 having a greater height, and thus volume and slope, than its neighbors. The dome Du3 is about the same diameter, but much less steep (~0.9°) and more like a swell than a classical dome. The top table gives these measured quantities, and the bottom table shows the derived ones from models of magma rise and eruption. One of the most interesting - and understandable - quantities is Te, the inferred duration of eruption, which ranges from 3 months to nearly 5 years. Careful perusers will note that the eruption durations are proportional to erupted volumes, which makes sense. To find out what all the other columns of data mean see the full paper by Raffeallo Lena and his coauthors. Here is a general overview of this professional work on domes. Note that these Undarum results are based on images by people well known to LPOD readers: Stefan Lammel, Paolo Lazzarotti and Bob Pilz, and coordinates were determined using Jim Mosher's LTVT software.

Chuck Wood

Related Links
Rükl plate 38



COMMENTS
To post comments regarding this LPOD you need to first register for the wiki by clicking the "Join this space" link under the Full Moon icon in the upper left corner of the screen, and wait for your membership to be approved. Once registered, you may still need to "Sign In" (link at top right of screen) to remove the "Protected" icon from the top of the LPOD page. Once you don't see a "Protected" icon, please click here and enter your comment in the space below. Please do not edit the LPOD itself!

1.